Detection of the γ-ray emission from the X-Ray nova GRO J0422+32

Details Detection of the γ-ray emission from the X-Ray nova GRO J0422+32 Detection of the γ-ray emission from the X-Ray nova GRO J0422+32

Jan 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002aspc..261..637i&link_type=abstract

The Physics of Cataclysmic Variables and Related Objects, ASP Conference Proceedings, Vol. 261. Edited by B. T. Gänsicke, K. Beu

Physics

Scientific paper

The evolution of the γ-ray emission from GRO J0422+32 was followed by COMPTEL since its discovery outburst of August 1992 till August 1997, and for 3 observations preceding the nova outburst. It was found that the GRO J0422+32 γ-ray emission is mostly confined to the energies between 1.5 and 2.0 MeV. This emission is prominent during observations that correspond to phases between 0.0 and 0.5 of the nova ~120 day periodical activity.

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